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    A joint radio gamma-ray variability study of the crab pulsar

    Access Status
    Fulltext not available
    Authors
    Jones, G.
    Shannon, Ryan
    Date
    2011
    Type
    Conference Paper
    
    Metadata
    Show full item record
    Citation
    Jones, G. and Shannon, R. 2011. A joint radio gamma-ray variability study of the crab pulsar, in Torres, D. and Rea, N. (ed), in Proceedings of the First Session of the Sant Cugat Forum on Astrophysics, Apr 12-16 2011, pp. 213-217. Barcelona: Springer-Verlag .
    Source Title
    Astrophysics and Space Science Proceedings
    DOI
    10.1007/978-3-642-17251-9_17
    ISSN
    1570-6591
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/59380
    Collection
    • Curtin Research Publications
    Abstract

    In order to understand pulsar emission, and coherent emission processes in general, it is important to assess the relationship between high energy and radio emission. Gamma-ray radio correlations can be used to test whether observed radio variability is solely the result of modifications to the radio emission processes (e.g., non-linear wave propagation [1]) or associated with bulk changes in the pulsar magnetosphere and charged particle flow (e.g., [2] and [3]). In the former case, gamma-ray emission would not be correlated with radio variability, but in the latter case, a pronounced correlation between gamma-rays would be expected. Giant radio pulses from the Crab pulsar [4] provide the best opportunity to study this relationship because they occur relatively frequently and provide a non-stationary signal which can be correlated against the high energy emission.

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